All Figures

	Figure 1: ACS HRC F330W image ( left panels), GALFIT model ( center panels) and residuals ( right panels) of our sample. Arrows indicate the direction of the radio source. The dashed lines in 1443+77 sketch the arc of emission mentioned in Sect. 4.1.
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In the text

	Figure 1: continued.
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In the text

	Figure 2: UV luminosity and radio power of the combined sample of GPS/CSS and FR I, FR II from Allen et al. (2002). The solid line shows the correlation between UV luminosity and radio power for GPS sources.
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In the text

	Figure 3: Difference between the UV and radio position angles (alignment) of the GPS and CSS galaxies versus radio size.
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In the text

	Figure 4: As Fig. 2, for radio size.
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In the text

	Figure 5: As Fig. 3, for UV luminosity.
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In the text

	Figure 6: UV size and radio size of GPS and CSS sources. The dashed line marks the locus of sources with equal radio and UV sizes.
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In the text

	Figure 7: Ratio of radio and UV sizes versus the alignment of the GPS and CSS sources. The dashed line marks the locus for sources with same UV and radio size and highest alignment i.e. where the radio source is most likely affecting the star formation in the host.
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In the text

	Figure 8: As Fig. 2, for redshift.
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In the text

	Figure 9: As Fig. 3, for radio power.
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In the text

	Figure 10: As Fig. 3, for redshift.
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In the text